Distance and reddening of the Local Group dwarf irregular galaxy NGC 6822
arXiv:1210.6753 · doi:10.1051/0004-6361/201220554
Abstract
On the basis of a new photometric analysis of the Local Group dwarf irregular galaxy NCG 6822 based on observations obtained with the Advanced Camera for Surveys onboard the Hubble Space Telescope, we have obtained a new estimate of the extinction of two fields located in the southeast region of the galaxy. Because of significant differences in the distance estimates to NGC 6822 available in literature, we decided to provide an independent determination of the distance to this galaxy based on an updated and self-consistent theoretical calibration of the tip of the red giant branch brightness. As a result we newly determined the distance to NGC 6822 to be equal to , and compared our measurement with the most recent determinations of this distance.
5 pages, 5 figures, Astronomy & Astrophysics (Research Note), in press (proof correction included)
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- Astrophysical Distance Scale II. Application of the JAGB Method: A Nearby Galaxy Sample
- Euclid: Early Release Observations -- Deep anatomy of nearby galaxies
- Carbon stars as standard candles: II. The median J magnitude as a distance indicator
- Ca II triplet spectroscopy of RGB stars in NGC 6822: kinematics and metallicities
- Carbon stars as standard candles -- III. Un-binned maximum likelihood fitting and comparison with TRGB estimations
- A state-of-the-art analysis of the dwarf irregular galaxy NGC 6822
- Euclid: Early Release Observations -- The star cluster systems of the Local Group dwarf galaxies IC 10 and NGC 6822
- Consistencies and inconsistencies in redshift-independent distances
- Evidence for Photometric Contamination in Key Observations of Cepheids in the Benchmark Galaxy IC 1613
- The dwarf irregular galaxy NGC 6822. II. Young, intermediate and old stellar populations: comparison between theory and observations
- On the dwarf irregular galaxy NGC 6822. I. Young, intermediate and old stellar populations